SPIRAL ROTATION IN RAYLEIGH-BENARD CONVECTION

(simulation of the Swift-Hohenberg equation coupled with mean flow)


Spiral terminated by a dislocation

Snapshots every 10 units of time:

Here is a movie (50 kB) of spiral rotation. Watch how the spiral quickly winds up first, and then the frequency of core rotation becomes smaller than dislocation's.


lev@gibbs.ucsd.edu